Transit planner
Predicted mid-transit times of the candidates in a chosen window, for observers planning follow-up photometry. The predictions were committed before the observations: for a planet, each transit should appear at the predicted time with the fitted depth.
A 1σ value in amber is longer than the transit duration, so the window for the start of the transit is wider than the transit itself. The TESS sector is filled in only when the transit falls inside a published TESS orbit window and the star is on a detector (README).
Assumptions
The times come from the repository's predictions.csv, which assumes a constant period (a linear ephemeris). The 1σ uncertainty is propagated from the period and epoch errors by the authors' predict.py; transit-timing variations would move transits away from these times. Times are UTC at Earth's centre, as described in the README. These are candidates, so a transit may not occur or may be too shallow to detect.
The prediction files were written when each candidate was registered (from 10 October 2026) and cover transits through June 2027; they are not recomputed here. Rows in tiers that are no longer counted keep their entries and can be shown with the options above. Radius, depth, Tmag and coordinates come from ephemerides.csv.